Hit papers significantly outperform the citation benchmark for their cohort. A paper qualifies
if it has ≥500 total citations, achieves ≥1.5× the top-1% citation threshold for papers in the
same subfield and year (this is the minimum needed to enter the top 1%, not the average
within it), or reaches the top citation threshold in at least one of its specific research
topics.
H0LiCOW – V. New COSMOGRAIL time delays of HE 0435−1223:H0to 3.8 per cent precision from strong lensing in a flat ΛCDM model
2016286 citationsF. Courbin, Dominique Sluse et al.profile →
H0LiCOW – IX. Cosmographic analysis of the doubly imaged quasar SDSS 1206+4332 and a new measurement of the Hubble constant
2019243 citationsF. Courbin, Dominique Sluse et al.profile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
hero ref
This map shows the geographic impact of G. Meylan's research. It shows the number of citations coming from papers published by authors working in each country. You can also color the map by specialization and compare the number of citations received by G. Meylan with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites G. Meylan more than expected).
This network shows the impact of papers produced by G. Meylan. Nodes represent research fields, and links connect fields that are likely to share authors. Colored nodes show fields that tend to cite the papers produced by G. Meylan. The network helps show where G. Meylan may publish in the future.
Co-authorship network of co-authors of G. Meylan
This figure shows the co-authorship network connecting the top 25 collaborators of G. Meylan.
A scholar is included among the top collaborators of G. Meylan based on the total number of
citations received by their joint publications. Widths of edges
represent the number of papers authors have co-authored together.
Node borders
signify the number of papers an author published with G. Meylan. G. Meylan is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Lemson, Gerard, M. Meneghetti, G. Meylan, Margarita Petkova, & S. Pires. (2014). A PCA-based automated finder for galaxy-scale strong lenses.24 indexed citations
Léon, S., G. Meylan, & F. Combes. (2000). Tidal tails around 20 Galactic globular clusters. Observational evidence for gravitational disk/bulge shocking. A&A. 359. 907–931.4 indexed citations
9.
Burud, I., F. Courbin, C. Lidman, et al.. (1998). RX J0911.4+0551: a complex quadruply imaged gravitationally lensed QSO.. Open Repository and Bibliography (University of Liège). 92. 29–32.3 indexed citations
10.
Meylan, G.. (1995). QSO absorption lines : proceedings of the ESO workshop held at Garching, Germany, 21-24 November 1994. Springer eBooks.2 indexed citations
11.
Meylan, G., et al.. (1994). ESO/OHP Workshop Dwarf Galaxies, Observatoire de Haute-Provence, France, 6-9 September 1993 : proceedings.8 indexed citations
12.
Meylan, G. & C. Pryor. (1993). Observational Constraints on the Internal Dynamics of Globular Clusters. ASPC. 50. 31–64.
13.
Binggeli, B., G. Meylan, & Ph. Prugniel. (1993). ESO/OHP Workshop on Dwarf Galaxies. Msngr. 74. 36–36.42 indexed citations
14.
Meylan, G., P. Dubath, & M. Mayor. (1991). Core Velocity Dispersion in High - Concentration Globular Clusters. Bulletin of the American Astronomical Society. 23. 833.1 indexed citations
15.
Vallenari, A., et al.. (1991). Star clusters of the large magellanic cloud. III. CCD-photometry of NGC 2164. Astronomy & Astrophysics Supplement Series. 87(3). 517–540.1 indexed citations
16.
Dubath, P., G. Meylan, M. Mayor, & Pierre Magain. (1990). Core velocity dispersion and mass-to-light ratio of the old Magellanic globular cluster NGC 1835. Open Repository and Bibliography (University of Liège).1 indexed citations
17.
Meylan, G., S. G. Djorgovski, N. Weir, & P. A. Shaver. (1990). PHL 1222 - an interacting quasar pair?. CaltechAUTHORS (California Institute of Technology). 59. 47–49.7 indexed citations
18.
Meylan, G. & G. Burki. (1986). RR Lyrae, Delta Scuti, SX Phoenicis stars and the Baade-Wesselink method.. The Messenger. 43. 16–23.1 indexed citations
19.
Meylan, G. & M. Mayor. (1985). Kinematical and Dynamical Properties of ω Cen and 47 Tuc. Bulletin of the American Astronomical Society. 17. 882.1 indexed citations
20.
Meylan, G. & B. Hauck. (1981). Relations between some photometric temperature parameters. Astronomy & Astrophysics Supplement Series. 46. 281–303.1 indexed citations
Rankless uses publication and citation data sourced from OpenAlex, an open and comprehensive
bibliographic database. While OpenAlex provides broad and valuable coverage of the global
research landscape, it—like all bibliographic datasets—has inherent limitations. These include
incomplete records, variations in author disambiguation, differences in journal indexing, and
delays in data updates. As a result, some metrics and network relationships displayed in
Rankless may not fully capture the entirety of a scholar's output or impact.